||These files are used in the dark current subtraction for WFC UVIS products from the following dates 02 March 2017 to 11 March 2017.
||STIS time dependent sensitivities are monitored and updated periodically as needed. Additionally, updated temperature dependent sensitivities have been calculated for the FUV MAMA and CCD detectors. Updated sensitivities will affect data taken after May 01, 2009. Changes are modest at longer wavelengths and older observations but are significant for recent observations at the shortest wavelengths.
||These files are used in the dark current subtraction for WFC/UVIS products from 11 February 2017 to 01 March 2017.
||The reason is that new STIS darks and bias files as well as a new ACS/WFC MDRIZTAB were delivered.